The Law of Star Formation in Disk Galaxies

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Scientific paper

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Star Formation, Star Formation Rate

Scientific paper

Does the available Hα-data from disk galaxies allow to distinguish between a SFR depending only on local current gas density and a more complicated SFR which also depends on galactocentric distance? What do the gas fractions tell us? These questions are answered with a practical Bayesian method we developed and which might be useful to address similar questions in other types of galaxies.

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